J/A+A/365/409       ISO continuum observations of quasars (Oyabu+, 2001)

ISO continuum observations of quasars at z=1-4. I. Spectral energy distributions of quasars from UV to far-infrared Oyabu S., Kawara K., Tsuzuki Y., Sofue Y., Sato Y., Okuda H., Taniguchi Y., Shibai H., Gabriel C., Hasegawa T. and Nishihara E. <Astron. Astrophys. 365, 409 (2001)> =2001A&A...365..409O 2001A&A...365..409O
ADC_Keywords: QSOs ; Infrared sources ; Photometry, VRI ; Photometry, infrared Mission_Name: ISO Keywords: infrared: galaxies - infrared: ISM: continuum - quasars: general - galaxies: photometry Abstract: Eight luminous quasars with -30<MB←27 at z=1.4-3.7 have been observed in the mid- and far-infrared using ISO. All the quasars have been detected in the mid-infrared bands of ISOCAM, while no far-infrared detections have been made with ISOPHOT. SEDs (Spectral Energy Distributions) from the UV to far-infrared have been obtained while supplementing ISO observations with photometry in the optical and near-infrared made from the ground within 17 months. The SEDs are compared with the MED (Mean spectral Energy Distributions) of low-redshift quasars with -27<MB←22. It is shown that our far-infrared observations were limited by confusion noise due to crowded sources. Description: File table3 contains the flux of quasars at high-redshift observed with ISO. File table4 contains the magnitude of them observed from the ground. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table3.dat 76 8 List of ISO flux if quasars table4.dat 92 7 List of optical and near-infrared magnitudes -------------------------------------------------------------------------------- See also: J/MNRAS/238/1171 : Optical/IR obs. of Radio Galaxies and QSOs (Dunlop+, 1989) Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 A12 --- Name Name of the source 14- 17 F4.2 mJy LW2 LW2 (6.7µm) flux 19- 22 F4.2 mJy e_LW2 Error of LW2 flux 24- 27 F4.1 mJy LW3 ? LW3 (14.3µm) flux 29- 32 F4.2 mJy e_LW3 ? Error of LW3 flux 34- 37 F4.2 mJy LW10 ? LW10 (12.0µm) flux 39- 42 F4.2 mJy e_LW10 ? Error of LW10 flux 44- 47 F4.1 mJy C90 ? C90 (90µm) flux 49- 50 I2 mJy e_C90 ? Error of C90 flux 52- 56 F5.1 mJy C160 C160 (170µm) flux 58- 60 I3 mJy e_C160 Error of C160 flux 62- 66 F5.1 10+13solLum LUVO UVO (0.1µm to 1µm) luminosity 68 A1 --- l_LIR Limit flag on LIR 69- 71 I3 10+13solLum LIR (1.5µm to 100µm) IR luminosity 73- 76 F4.1 10+13solLum L1.25 1.25 micron luminosity -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 A12 --- Name Name of the source 14- 18 F5.2 mag Vmag ? V magnitude 20- 23 F4.2 mag e_Vmag ? rms uncertainty on Vmag 25- 29 F5.2 mag Rmag ? R magnitude 31- 34 F4.2 mag e_Rmag ? rms uncertainty on Rmag 36- 40 F5.2 mag Imag ? I magnitude 42- 45 F4.2 mag e_Imag ? rms uncertainty on Imag 47- 51 F5.2 mag Jmag ? J magnitude 53- 56 F4.2 mag e_Jmag ? rms uncertainty on Jmag 58- 62 F5.2 mag Hmag ? H magnitude 64- 67 F4.2 mag e_Hmag ? rms uncertainty on Hmag 69- 73 F5.2 mag K'mag ? K' magnitude 75- 78 F4.2 mag e_K'mag ? rms uncertainty on K'mag 80- 87 A8 "YY/MM/DD" ObsDate Universal time when observed 89- 92 A4 --- Tel Observed telescope (1) -------------------------------------------------------------------------------- Note (1): The following abbreviations are used: Kiso: the 1m Schmidt telescope at the Kiso observatory OAO: the 1.88m telescope at Okayama Astrophysical Observatory CTIO: the 0.9m telescope at CTIO -------------------------------------------------------------------------------- Acknowledgements: S. Oyabu
(End) Patricia Bauer [CDS] 27-Oct-2000
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line